Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Analysis of the Giacobini-Zinner bow wave

Conference ·
OSTI ID:6839100
The cometary bow wave of P/Giacobini-Zinner has been analyzed using the complete set of ICE field and particle observations to determine if it is a shock. Changes in the magnetic field and plasma flow velocities from upstream to downstream have been analyzed to determine the direction of the normal and the propagation velocity of the bow wave. The velocity has then been compared with the fast magnetosonic wave speed upstream to derive the Mach number and establish whether it is ''supersonic'', i.e., a shock, or ''subsonic,'' i.e., a large amplitude wave. The various measurements have also been compared with values derived from a Rankine-Hugoniot analysis. The results indicate that, inbound, the bow wave is a shock with M = 1.5. Outbound, a subsonic mach number is obtained, however, arguments are presented that the bow wave is also likely to be a shock at this location. 11 refs., 4 figs., 2 tabs.
Research Organization:
Los Alamos National Lab., NM (USA); Jet Propulsion Lab., Pasadena, CA (USA); Imperial Coll. of Science and Technology, London (UK); Maryland Univ., College Park (USA); National Aeronautics and Space Administration, Greenbelt, MD (USA). Goddard Space Flight Center; European Space Research and Technology Centre, Noordwijk (Netherlands)
DOE Contract Number:
W-7405-ENG-36
OSTI ID:
6839100
Report Number(s):
LA-UR-87-40; CONF-8610207-7; ON: DE87005121
Country of Publication:
United States
Language:
English

Similar Records

Subcritical dispersive shock waves upstream of planetary bow shocks and at comet Giacobini-Zinner
Journal Article · Sat Oct 01 00:00:00 EDT 1988 · Geophys. Res. Lett.; (United States) · OSTI ID:7088416

Plasma parameters near the comet Halley bow shock
Journal Article · Fri Nov 30 23:00:00 EST 1990 · Journal of Geophysical Research; (United States) · OSTI ID:5378826

New plasma physics lab at Giacobini-Zinner. [Comet]
Journal Article · Tue Oct 01 00:00:00 EDT 1985 · Science (Washington, D.C.); (United States) · OSTI ID:5733074